We invite abstract submissions for the session ‘Latest Trends In Observing And Understanding The Dynamics Of The Solar Atmosphere: From MHD Waves To Small-Scale Transients’ which will take place at NAM2017.

The Sun is a highly structured and dynamic body, containing a wide range of waves, instabilities, and more transient, sometimes explosive, phenomena (e.g., Ellerman bombs, swirls, spicules). This session will highlight and discuss recent improvements in our understanding of the dynamics of the solar atmosphere including: (i) how transient events are driven; (ii) the detection, interpretation, and analysis of MHD waves in solar wave-guides; (iii) what MHD waves can tell us about the local background plasma properties (through techniques such as solar magneto-seismology).

The deadline for abstract submission is April 14, 2017.
More information can be found at the conference website: https://nam2017.org/